[PDF] Top 20 Numerical relativity and the early Universe
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Numerical relativity and the early Universe
... We designed and debugged a software for numerical simulations in gravity with scalar fields. The main di ff erence from previous works is the special ansatz for the metric and hence slightly di ff erent concept with ... See full document
6
Is the Cosmological Constant, a “Vacuum” Field? We Explore This by Squeezing Early Universe “Coherent Semi Classical States”, and Compare This to Energy from the Early Universe Heisenberg Uncertainty Principle
... GW. Early universe models with g ∗ ~ 1000 or so are not in the realm of observational science, yet, according to Hector De La Vega (2009) in personal communications with the author,) at the Colmo, Italy ... See full document
17
Chameleons in the early universe: kicks, rebounds, and particle production
... Light scalar fields are of great interest in cosmology because they arise in many explanations for the current acceleration of the expansion of the Universe [1–5]. It is challenging for these models to evade the ... See full document
28
Turbulence of weak gravitational waves in the early universe
... the Universe quasiuniformly rather than being concentrated locally in space and time near an isolated burst event, and it is likely that their distribution was broad in frequencies and propagation ...the ... See full document
7
Spectrally accurate initial data in numerical relativity
... the universe like waves on a ...the universe, such as how stars die, the birth of black holes, and how the universe evolved into what it is ...of Relativity is ... See full document
163
Early Universe and Evolution of the Present Universe: Exact Solution Models
... general relativity G plays the role of a coupling constant between geometry and matter in Einstein’s field ...the early stage of the evolution of the ... See full document
9
Some Numerical Curiosities about the Universe
... the numerical connection among Equations (13), (20) and ...a numerical linkage between one parameter belonging to Quantum mechanics, ...General relativity as Einstein’s gravi- tational constant ... See full document
8
Numerical Relativity beyond General Relativity
... general relativity in the non-linear, dynamical, strong-field regime of gravity is one of the major goals of gravitational wave ...general relativity (GR) requires numerical inspiral, merger, and ... See full document
249
Relativity of Speed of Light with Speed of Universe Expansion
... Cosmic background radiation is well explained as radiation left over from an early stage in the development of the universe, and its discovery is considered a landmark test of the Big Bang model of the ... See full document
9
A PRECISE STUDY OF GRAVITATIONL FORCE
... the Universe, possibly in the form of quantum gravity, supergravity or a gravitational singularity, along with ordinary space and time, developed during the Planck epoch (up to 10−43 seconds after the birth of the ... See full document
7
Black Hole Simulations: From Supercomputers to Your Laptop
... the early inspiral region where the surrogate depends on the hybridization ...the early inspiral and the hybridization errors are smaller than or comparable to the NR resolution error for these ... See full document
261
Origin of the Universe, Dark Energy, and Dark Matter
... our universe is de- scribed by the finite number of bits of information on the horizon from which a light signal could ever reach the ...expanding universe such as ours, all of the universe was once ... See full document
19
Optimization of Finite-Differencing Kernels for Numerical Relativity Applications
... Multi-thread performances (left panel) and speedup (right panel) for block size n = 128 as a function of the number of threads, in the case of the wave equations with stencil size S = 2.[r] ... See full document
10
Conformality Lost: Broken Symmetries in the Early Universe
... our universe inflated for a sufficiently long time to account for present ...the universe must be smooth on a patch larger than its Hubble radius [75], but these are rather unnatural initial ... See full document
165
A new paradigm for the dynamics of the early Universe
... the Universe is best formulated in terms of a series of successive approximations based on a viable cosmography derived from current observations with a minimum number of phenomenological constraints on the ... See full document
36
Gravitino condensates in the early universe and inflation
... point of view, the scalar curvature-squared terms in (27) are viewed as the result of quantum fluc- tuations (at one-loop level) of conformal (massless or high energy) matter fields of various spins, which have been ... See full document
17
The photometric properties of galaxies in the early Universe
... Our ability to probe the very high redshift ( z ∼ 7 and beyond) Universe has been dramatically transformed in recent years. This transformation is thanks largely to the wealth of observations ob- tained by the ... See full document
10
Interacting Holographic Dark Energy in Bianchi Type V Universe with Variable Deceleration Parameter
... Motivated by these investigations, we have constructed spatially homogeneous and anisotropic Bianchi type-V universe field with interacting dark matter and holographic dark energy. In this paper, we obtained the ... See full document
11
Mach’s Principle to Hubble’s Law and Light Relativity
... the universe can alter the inertia of the object at ...the universe or spacetime. The disturbed universe or distorted spacetime will then act/affect back on the moving object to vary its inertia or ... See full document
10
Introducing Numerical Analyses in the Early Phases of the Design Process
... this early phase of a products life cycle is usually imprecise, approximate or unknown, the designers decision-making is a very demanding ...the numerical models are based on many suppositions and ... See full document
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